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21#
發(fā)表于 2025-3-25 03:19:34 | 只看該作者
22#
發(fā)表于 2025-3-25 08:15:31 | 只看該作者
Backreaction of Quantum Gravitational Modes,tive energy-momentum tensor is computed and we show that it has a non-zero trace that contributes to the cosmological constant. By confronting our result with LIGO’s data, the first constraint on the amplitude of the massive mode is obtained: ..
23#
發(fā)表于 2025-3-25 12:11:48 | 只看該作者
24#
發(fā)表于 2025-3-25 16:39:12 | 只看該作者
Sakshi Thakur,Vishal Mutreja,Ajay Sharmal, thus stabilizing the electroweak vacuum. For specific values of the Higgs field initial condition and of its non-minimal coupling, the inflaton can quickly drive the Higgs field to the electroweak vacuum during inflation.
25#
發(fā)表于 2025-3-25 22:47:19 | 只看該作者
26#
發(fā)表于 2025-3-26 01:52:51 | 只看該作者
Dynamic Modes of Atomic Force Microscopyhese modes be excited in strong astrophysical processes, such as black hole mergers, creating gravitational waves. We analyze the significance for gravitational wave events such as GW 150914 recently observed by the Advanced LIGO collaboration.
27#
發(fā)表于 2025-3-26 07:30:23 | 只看該作者
Gravitational Waves in Quantum Gravity,hese modes be excited in strong astrophysical processes, such as black hole mergers, creating gravitational waves. We analyze the significance for gravitational wave events such as GW 150914 recently observed by the Advanced LIGO collaboration.
28#
發(fā)表于 2025-3-26 10:59:58 | 只看該作者
29#
發(fā)表于 2025-3-26 15:21:45 | 只看該作者
CFD Investigation into the Wave Added Resistance of Two Shipsesistance and propulsion characteristics in calm water as well as in the wave conditions encountered service. In this process CFD has become quite mature in quantifying the frictional and pressure drag in the calm water. In waves, CFD simulations are still less time efficient compared to potential f
30#
發(fā)表于 2025-3-26 20:05:16 | 只看該作者
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